Spectral modeling in the VNIR range of 67P/Churyumov-Gerasimenko nucleus from VIRTIS-M onboard Rosetta

Raponi, A. and Ciarnello, M. and Capaccioni, F. and Filacchione, G. and De Sanctis, M.C. and Erard, S. and Leyrat, C. and Bockelee-Morvan, D. and Tosi, F. and Capria, M. T. and Piccioni, G. and Palomba, E. and Longobardo, A and Drossart, P. and Quirico, E. and Beck, P. and Schmitt, B. and Barucci, Antonella and Arnold, Gabriele and Blecka, M. (2015) Spectral modeling in the VNIR range of 67P/Churyumov-Gerasimenko nucleus from VIRTIS-M onboard Rosetta. In: 10th European Planetary Science Congress (EPSC), 10, p. 573. European Planetary Science Congress 2015, 2015-09-27 - 2015-10-02, Nantes, France.

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Official URL: http://meetingorganizer.copernicus.org/EPSC2015/EPSC2015-573.pdf

Abstract

Topic of this work is the analysis of the surface composition of comet 67P/Churyumov-Gerasimenko using the data obtained by the VIRTIS instrument onboard the Rosetta spacecraft. We have focused on the VNIR spectral range (0.4 - 2.5 μm) which presents a nearly flat spectrum with quite uniform spectral slopes across the entire comet surface. In this work we report about the spectral modeling of CG VIS-IR spectra by means of Hapke’s radiative transfer model.

Item URL in elib:

https://elib.dlr.de/100887/

Document Type:

Conference or Workshop Item (Speech)

Title:

Spectral modeling in the VNIR range of 67P/Churyumov-Gerasimenko nucleus from VIRTIS-M onboard Rosetta

Authors:

Authors	Institution or Email of Authors	Author's ORCID iD	ORCID Put Code
Raponi, A.	INAF-IASF, Italy	UNSPECIFIED	UNSPECIFIED
Ciarnello, M.	INAF-IASF, Italy	UNSPECIFIED	UNSPECIFIED
Capaccioni, F.	INAF-IASF, italy	UNSPECIFIED	UNSPECIFIED
Filacchione, G.	INAF-IASF, Rome, Italy	UNSPECIFIED	UNSPECIFIED
De Sanctis, M.C.	Istituto Nazionale di Astrofisica, Rome, Italy.	UNSPECIFIED	UNSPECIFIED
Erard, S.	LESIA	UNSPECIFIED	UNSPECIFIED
Leyrat, C.	LESIA	UNSPECIFIED	UNSPECIFIED
Bockelee-Morvan, D.	Observatoire de Paris, Meudon	UNSPECIFIED	UNSPECIFIED
Tosi, F.	INAF-IASF Istituto di Astrofisica Spaziale e Fisica Cosmica, Roma Italy	UNSPECIFIED	UNSPECIFIED
Capria, M. T.	Instituto di Astrofisica Spaziale e Fisica Cosmica, Roma, Italy	UNSPECIFIED	UNSPECIFIED
Piccioni, G.	INAF-IASF	UNSPECIFIED	UNSPECIFIED
Palomba, E.	Institute for Interplanetary Space Physics - INAF, Rome, Italy	UNSPECIFIED	UNSPECIFIED
Longobardo, A	INAF-LAPS, Via del Fosso del Cavaliere 100, I-00133 Rome, Italy	UNSPECIFIED	UNSPECIFIED
Drossart, P.	Observatoire de Paris, Meudon, France	UNSPECIFIED	UNSPECIFIED
Quirico, E.	Laboratory of Planetology, CNRS Joseph Fourier University	UNSPECIFIED	UNSPECIFIED
Beck, P.	Laboratoire de Planétologie de Grenoble (LPG) - University Joseph Fourier Grenoble, Grenboble, France	UNSPECIFIED	UNSPECIFIED
Schmitt, B.	Grenoble Planetology Laboratory	UNSPECIFIED	UNSPECIFIED
Barucci, Antonella	Observatoire de Paris-Meudon, France	UNSPECIFIED	UNSPECIFIED
Arnold, Gabriele	UNSPECIFIED	UNSPECIFIED	UNSPECIFIED
Blecka, M.	Polish Academi of Sciences, Warsaw, Poland	UNSPECIFIED	UNSPECIFIED

Date:

29 September 2015

Journal or Publication Title:

10th European Planetary Science Congress (EPSC)

Refereed publication:

Open Access:

Yes

Gold Open Access:

In SCOPUS:

In ISI Web of Science:

Volume:

Page Range:

p. 573

Series Name:

EPSC Abstracts

Status:

Published

Keywords:

VIRTIS, Rosetta, 67P, spectral modeling

Event Title:

European Planetary Science Congress 2015

Event Location:

Nantes, France

Event Type:

international Conference

Event Start Date:

27 September 2015

Event End Date:

2 October 2015

Organizer:

Europlanet

HGF - Research field:

Aeronautics, Space and Transport

HGF - Program:

Space

HGF - Program Themes:

Space Exploration

DLR - Research area:

Raumfahrt

DLR - Program:

R EW - Space Exploration

DLR - Research theme (Project):

R - Project ROSETTA Instruments (old)

Location:

Berlin-Adlershof

Institutes and Institutions:

Institute of Planetary Research > Leitungsbereich PF

Deposited By:

Kappel, David

Deposited On:

17 Dec 2015 08:20

Last Modified:

24 Apr 2024 20:06

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